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NRAO Home > CASA > CASA Cookbook and User Reference Manual |
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8.4 Single Dish Imaging
Single dish imaging is supported within CASA using standard tasks and tools. The data must be in the Measurement Set format. Once there, you can use the im (imager) tool to create images:
Tool example:
scans.save(’outputms’,’MS2’) # Save your data from ASAP into an MS
im.open(’outputms’) # open the data set
im.selectvis(nchan=901,start=30,step=1, # choose a subset of the data
spwid=0,field=0) # (just the key emission channels)
dir=’J2000 17:18:29 +59.31.23’ # set map center
im.defineimage(nx=150,cellx=’1.5arcmin’, # define image parameters
phasecenter=dir,mode=’channel’,start=30, # (note it assumes symmetry if ny,celly
nchan=901,step=1) # aren’t specified)
im.setoptions(ftmachine=’sd’,cache=1000000000) # choose SD gridding
im.setsdoptions(convsupport=4) # use this many pixels to support the
# gridding function used
# (default=prolate spheroidal wave function)
im.makeimage(type=’singledish’, # make the image
image=’FLS3a_HI.image’)
im.open(’outputms’) # open the data set
im.selectvis(nchan=901,start=30,step=1, # choose a subset of the data
spwid=0,field=0) # (just the key emission channels)
dir=’J2000 17:18:29 +59.31.23’ # set map center
im.defineimage(nx=150,cellx=’1.5arcmin’, # define image parameters
phasecenter=dir,mode=’channel’,start=30, # (note it assumes symmetry if ny,celly
nchan=901,step=1) # aren’t specified)
im.setoptions(ftmachine=’sd’,cache=1000000000) # choose SD gridding
im.setsdoptions(convsupport=4) # use this many pixels to support the
# gridding function used
# (default=prolate spheroidal wave function)
im.makeimage(type=’singledish’, # make the image
image=’FLS3a_HI.image’)
More information about CASA may be found at the
CASA web page
Copyright © 2010 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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